Object | Sp. Type | Ref. | V | ![]() |
b-y | ![]() |
m1 | ![]() |
c1 | ![]() |
N(uvby) | ![]() |
![]() |
N(![]() |
BK Peg | F8a | C10 | 9.982 | 7 | 0.362 | 6 | 0.143 | 12 | 0.456 | 12 | 176 | 2.639 | 7 | 9 |
C10 | 10.463 | 4 | 0.369 | 7 | 0.136 | 11 | 0.477 | 4 | 6 | |||||
HD 222249 | F5 IVb | C10 | 7.146 | 6 | 0.309 | 4 | 0.177 | 8 | 0.503 | 8 | 118 | 2.645 | 3 | 8 |
O83 | 7.139 | 5 | 0.317 | 3 | 0.158 | 4 | 0.503 | 4 | 1 | |||||
O94 | 7.151 | 9 | 0.317 | 3 | 0.161 | 3 | 0.507 | 2 | 3 | 2.645 | 8 | 3 | ||
P69 | 7.010 | 0.303 | 0.190 | 0.487 | 2 | |||||||||
HD 222391 | G0 IIIc | C10 | 7.566 | 6 | 0.362 | 6 | 0.185 | 11 | 0.424 | 8 | 134 | 2.617 | 4 | 8 |
O83 | 7.559 | 5 | 0.371 | 3 | 0.170 | 4 | 0.420 | 5 | 1 | |||||
O94 | 0.372 | 3 | 0.167 | 4 | 0.427 | 6 | 1 | 2.620 | 6 | 2 | ||||
HD 223323 | F2 IV-Vd | C10 | 7.084 | 6 | 0.290 | 5 | 0.138 | 10 | 0.414 | 9 | 189 | 2.636 | 7 | 13 |
J96 | 7.076 | 4 | 0.302 | 1 | 0.123 | 1 | 0.407 | 1 | 9 | 2.640 | ||||
J96 | 7.094 | 2 | 0.300 | 0 | 0.128 | 5 | 0.409 | 4 | 2 | |||||
J96 | 7.089 | 1 | 0.299 | 0 | 0.120 | 0 | 0.406 | 1 | 2 | |||||
O83 | 7.080 | 6 | 0.296 | 5 | 0.124 | 5 | 0.412 | 4 | 4 | 2.643 | 5 | 4 |
References. (a) Popper (1983) (b) Harlan & Taylor (1970); (c) Heard (1956); (d) Harlan (1969).
Notes. C10
= This paper. J96 = Jordi et al. (1996).
O83 = Olsen (1983).
O94 = Olsen (1994).
P69 = Perry (1969).
For BK Peg, the
information by C10 is the mean value outside eclipses
(first line) and during the central part of secondary eclipse (second
line), where 98% (y) of the light of the secondary
component is eclipsed. N is the total number of observations used to
form the mean values, and
is the rms
error (per observation) in mmag.
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